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    1. http://www.arcetri.astro.it/igm50/posters_all/armillotta.pdf
    ... coronal gas but the efficiency of this phenomenon is significantly reduced at increasing coronal temperature. - takes place at the interface - cold metal-rich gas mixes with low-Z hot gas - the mixing can cause the cooling of the hot gas (Marinacci et al ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/igm50/posters_all/armillotta.pdf -- 1235.5 Кб -- 16.07.2015
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    2. http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ISM/NGC7027.txt
    ... Encircling this hot gas is a cloud of dust and cool molecular hydrogen gas that can ... The white is emission from the hot gas surrounding the central star; the red and ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ISM/NGC7027.txt -- 6.6 Кб -- 30.01.2001
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    3. http://www.arcetri.astro.it/~sperello/AIPC1035_218.pdf
    ... particularly in the massive ETG, where hot gas is denser Therefore Hi survival in ... which is thought to be due to hot gas swept back by the ram pressure caused by the ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~sperello/AIPC1035_218.pdf -- 790.3 Кб -- 17.10.2008
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    4. Hubble Provides Multiple Views of How to Feed a Black Hole (PRC98-14)
    ... dust mixed with cold hydrogen gas are silhouetted against the incandescent yellow-orange glow from hot gas and stars behind it ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Galassie/Cauldron.html -- 4.3 Кб -- 10.04.2001
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    5. http://www.arcetri.astro.it/~sperello/AA518_L50.pdf
    ... dust formation around evolved stars and its subsequent destruction in a hot gas ... has been observed by Chandra, and the central hot gas density estimated to be 0.011 ... We thus assume a hot gas density of 0.02 cm-3 for all our ETGs. ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~sperello/AA518_L50.pdf -- 133.2 Кб -- 19.07.2010
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    6. http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ISM/M57.txt
    ... clumps of material embedded in the gas at the edge of the nebula; the dying central star floating in a blue haze of hot gas ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ISM/M57.txt -- 2.4 Кб -- 30.01.2001
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    7. APOD: 2000 January 10 - Brown Sun Bubbling
    ... Explanation: Our Sun may look like all soft and fluffy, but its not. Our Sun is an extremely large ball of bubbling hot gas , mostly hydrogen gas. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/sun/sunhalpha_gendler_big.html -- 4.7 Кб -- 06.12.2000
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    8. http://www.arcetri.astro.it/~sperello/astroph0709.2096.pdf
    ... the massive ellipticals, contain large quantities of hot gas (T 107 K ), which can ... the effect of tidal encounters on hot gas flows, and found the creation of dense ... HI in Early Type Galaxies hot gas flows in quite flattened galaxies (S0 or flat ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~sperello/astroph0709.2096.pdf -- 154.5 Кб -- 13.09.2007
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    9. Hubble Provides Multiple Views of How to Feed a Black Hole (PRC98-14)
    ... of the nearest active galaxy to Earth, Centaurus A. Hubble's Near Infrared Camera and Multi-Object Spectrometer was used to peer past the dust to discover a tilted disk of hot gas at the galaxy's center (white bar running diagonally across image center ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Galassie/CentaurusA.html -- 3.4 Кб -- 10.04.2001
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    10. http://www.arcetri.astro.it/~sperello/AA474_851.pdf
    ... massive ellipticals, contain large quantities of hot gas (T 107 K), which can amount ... the effect of tidal encounters on hot gas flows, and found the creation of dense ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~sperello/AA474_851.pdf -- 168.6 Кб -- 26.10.2007
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